發布時間: 2021 Jul 15 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 15 Jul 2021 | 074 | 004 |
| 16 Jul 2021 | 076 | 001 |
| 17 Jul 2021 | 074 | 001 |
Solar activity was at very low levels, with only B-class flares produced in the last 24 hours. NOAA Active Region (AR) 2842 (Catania sunspot group 17) continues to decay, NOAA AR 2843 (Catania sunspot group 18) has lost some magnetic complexity, while NOAA 2841 has now become a plage region. For the next 24 hours the solar activity is expected to remain very low with a small change of a C-class flare.
No Earth directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph imagery.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold and is expected to remain below this level during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.
The High Speed Stream (HSS) initially predicted to arrive on July 11, arrived weakened at 09:00UT July 14 and had a minor effect on the solar wind. The solar wind speed increased from 340 to 440 km/s during the last 24 hours. The total magnetic field varied between 1 and 13 nT in the last 24 hours. The Bz was predominantly negative during the last 24 hours, with values varying between -12 and 6 nT. The interplanetary magnetic field phi angle was predominantly negative (directed towards the Sun) during the last 24 hours. The solar wind conditions are expected to reflect a slow solar wind regime for the next 24 hours.
Geomagnetic conditions were quiet to active both globally and locally (NOAA Kp index and K Dourbes 1-4) over the past 24 hours. This was due to the arrival of the HSS mentioned above. They are expected to be at quiet levels for the next 24 hours.
今日估計的國際太陽黑子數(ISN):017,基於17個觀測站。
| 卡塔尼亞沃爾夫數 | 037 |
| 10厘米太陽通量 | 072 |
| AK Chambon La Forêt | 021 |
| AK Wingst | 019 |
| 估計地磁Ap指數 | 018 |
| 估計國際太陽黑子數 | 027 - 基於21個觀測站 |
| 日 | 開始 | 最大值 | 結束 | 位置 | 強度 | OP | 10cm | 卡塔尼亞天體物理觀測站/美國國家海洋暨大氣管理局 | 電波爆發類型 | |
|---|---|---|---|---|---|---|---|---|---|---|
| 無 | ||||||||||
由太陽影響數據分析中心提供© - SIDC - 由 SpaceWeatherLive處理
所有時間均採用 UTC 時間
很多網友來到 SpaceWeatherLive 追蹤太陽活動或極光觀測機會,但隨著流量增加,維持伺服器運作的成本也隨之越高。若您喜歡 SpaceWeatherLive 並想支持這個計畫,可選擇訂閱無廣告版本,或考慮捐款。有了您的幫助,我們才能讓 SpaceWeatherLive 持續運作!
| 上一個 X-閃焰 | 08/12/2025 | X1.1 |
| 上一個 M-閃焰 | 21/12/2025 | M1.3 |
| 上一個 地球磁爆 | 21/12/2025 | Kp5 (G1) |
| 無黑子天數 | |
|---|---|
| 上一個無黑子日 | 08/06/2022 |
| 黑子數月平均 | |
|---|---|
| 11月 2025 | 91.8 -22.8 |
| 12月 2025 | 116.9 +25.1 |
| 過去 30 天內 | 109 +22.2 |